2014/06/30 by Jeremiah Birrell, Cheng Tao Yang, Cheng-Tao Yang +1
Mathematics · Physics and Astronomy · #Astrophysics #Boltzmann constant #Boltzmann equation #Computation #Cosmic microwave background #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Lepton #Mathematics #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Physics #Quantum mechanics #Solver #Statistical physics #Universe #Weinberg angle #astro-ph.CO #hep-ph #nucl-th
paper · pdf · doi:10.1016/j.nuclphysb.2014.11.020
published as Nucl. Phys. B 890, 481 (2015) · 38 pages, 14 figures
openalex publication_date 2014/11/29 · arxiv created 2014/12/12 · arxiv updated 2015/06/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Analysis of cosmic microwave background radiation fluctuations favors an effective number of neutrinos, Nν>3. This motivates a reinvestigation of the neutrino freeze-out process. Here we characterize the dependence of Nν on the Standard Model (SM) parameters that govern neutrino freeze-out. We show that Nν depends on a combination η of several natural constants characterizing the relative strength of weak interaction processes in the early Universe and on the Weinberg angle sin2θW. We determine numerically the dependence Nν(η,sin2θW) and discuss these results. The extensive numerical computations are made possible by two novel numerical procedures: a spectral method Boltzmann equation solver adapted to allow for strong reheating and emergent chemical non-equilibrium, and a method to evaluate Boltzmann equation collision integrals that generates a smooth integrand.